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A Semi-Implicit, Three-Dimensional Model for Estuarine ... - USGS

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26 A <strong>Semi</strong>-<strong>Implicit</strong>, <strong>Three</strong>-<strong>Dimensional</strong> <strong>Model</strong> <strong>for</strong> <strong>Estuarine</strong> Circulation<br />

and<br />

∂ ∂u<br />

------- ⎛ 1<br />

ν ------- ⎞ ∂ ∂u<br />

------- ⎛ 1<br />

∂x<br />

⎝ t ν ------- ⎞ ∂ ∂u1<br />

+<br />

1 ∂x<br />

⎠<br />

1 ∂x<br />

⎝ t + ------- ⎛ν------- ⎞<br />

2 ∂x<br />

⎠<br />

2 ∂x<br />

⎝ t<br />

3 ∂x<br />

⎠<br />

3<br />

(2.23)<br />

∂ ∂u<br />

------- ⎛ 2<br />

ν ------- ⎞ ∂ ∂u<br />

------- ⎛ 2<br />

∂x<br />

⎝ t<br />

ν ------- ⎞ ∂ ∂u2<br />

+<br />

1 ∂x<br />

⎠<br />

1 ∂x<br />

⎝ t + ------- ⎛ν------- ⎞<br />

2 ∂x<br />

⎠<br />

2 ∂x<br />

⎝ t . (2.24)<br />

3 ∂x<br />

⎠<br />

3<br />

The <strong>for</strong>m of 2.23 and 2.24 does not preserve the symmetry of the turbulent stress tensor because the right sides of<br />

– u1 ′ u′ 2 = νt( ∂u1 ⁄ ∂x2)<br />

and – u2 ′ u′ 1 = νt( ∂u2 ⁄ ∂x1)<br />

are no longer equal as they should be. For this reason, the <strong>for</strong>m of<br />

2.20 and 2.21 sometimes is preferred. It turns out, however, that the loss of symmetry in the stress tensor generally is not a serious<br />

concern <strong>for</strong> estuarine modeling.<br />

When 2.20 and 2.21 or 2.23 and 2.24 is introduced into equation 2.15, the problem of turbulence closure is shifted to that of<br />

defining the distribution of the eddy viscosity. Unlike the molecular viscosity, the eddy viscosity is not a fluid property but instead<br />

varies throughout the flow field as a function of the length and velocity scales of the turbulent eddies. Because the largest-scale<br />

eddies are primarily responsible <strong>for</strong> the turbulent transport of momentum and salt, these largest eddies influence most the magni-<br />

tude of v t. The geometry of the estuary determines to a great extent the size of the largest eddies. Because of the striking disparity<br />

between the length scales of the horizontal and vertical dimensions of most estuaries, the intensity and size of the horizontal eddies<br />

are much greater than those of the vertical eddies. The turbulent motions under these conditions are said to be anisotropic (direction<br />

dependent). It is typical to define separate horizontal and vertical eddy viscosities, A H and A V , to account <strong>for</strong> the anisotropy. The<br />

turbulent stress terms in the <strong>for</strong>m of 2.23 and 2.24 then become<br />

and<br />

∂ ∂u<br />

------- ⎛ 1<br />

A ------- ⎞ ∂ ∂u<br />

------- ⎛ 1<br />

∂x<br />

⎝ H<br />

A ------- ⎞ ∂ ∂u1<br />

+<br />

1 ∂x<br />

⎠<br />

1 ∂x<br />

⎝ H + ------- ⎛A------- ⎞<br />

2 ∂x<br />

⎠<br />

2 ∂x<br />

⎝ V<br />

(2.25)<br />

3 ∂x<br />

⎠<br />

3<br />

∂ ∂u<br />

------- ⎛ 2<br />

A -------- ⎞ ∂ ∂u<br />

------- ⎛ 2<br />

∂x ⎝ H<br />

A -------- ⎞ ∂ ∂u2 +<br />

1 ∂x ⎠<br />

1 ∂x ⎝ H + ------- ⎛A-------- ⎞<br />

2 ∂x ⎠<br />

2 ∂x ⎝ V . (2.26)<br />

3 ∂x ⎠<br />

3<br />

For estuaries, a possible range of magnitudes is 10 3 to 10 6 cm 2 /s <strong>for</strong> A H and 1 to 500 cm 2 /s <strong>for</strong> A V.<br />

Because of the large horizontal extent of flow in most estuaries, the horizontal variations in mean-flow quantities generally<br />

are much more gradual than the vertical variations. As a result, the four terms in 2.25 and 2.26 involving horizontal gradients of<br />

mean velocities ordinarily are much smaller than the two terms involving vertical gradients. (This will be demonstrated also in<br />

Section 2.5 using scale analysis.) Each of the terms in 2.25 and 2.26 represent momentum diffusion due to turbulence in addition<br />

to their interpretation as stresses. Horizontal momentum diffusion generally is less significant in estuaries than vertical momentum<br />

diffusion.

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